Physics

Physics, 22.07.2019 19:30, Claude512

What is the last nuclear fusion stage in the life of a low-mass star like the sun?

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Physics, 21.06.2019 17:10, 87haymaker

The “death throes” of stars are amongst the most complex phenomena in all of astronomy, and the “corpses” of stars amongst the most energetic and exotic objects in existence. beginning at the end of the core helium fusion stage in a star’s life, describe in detail the post-main sequence development of both (a) a 1.0 solar mass star, and (b) a 25.0 solar mass star. in what significant ways do they differ? what role does each of these types of stars play in the "star-gas-star" cycle and the evolution of chemical elements in our galaxy?

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Chemistry, 14.07.2019 08:00, adrianbanuelos1999

For a star of sun-like mass, what is the last stage of the nuclear fusion? a. hydrogen to helium b. helium to carbon and oxygen c. fusion goes all the way up to iron. d. carbon to magnesium

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Physics, 09.10.2019 20:30, alanadwhite48

The sun has a lifetime of approximately 10 billion years. if you could determine the rate of nuclear fusion for a star with twice the mass of the sun, which of the following would best describe how its fusion rate would compare to the sun? choose the best possible response to complete the sentence given below. a star with twice the mass of the sun would have a rate of nuclear fusion that is the rate of fusion in the sun. a) less than b) a little more than c) twice d) more than twice explain your reasoning for the choice you made.

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Chemistry, 09.10.2019 21:50, Mochalav6675

Arrange the events in the life of a star in the correct order.all that remains of the star now is the core. in some cases, the star turns into a black hole.as the nuclear fusion sets off a chain reaction, the nebula gets hotter and brighter and turns into a star.the star stays in the main sequence stage for a long time.the star runs out of hydrogen and turns into a planetary nebula or a supernova, depending on its mass.heavy elements are created when the supernova explodes.the temperature increases in the center of a nebula, and nuclei begin to fuse.

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